Arxiv Oai Expandedmetadata only
Thermodynamic-Geometric Phase Transition and Gravitational-Wave Quasinormal Modes of Schwarzschild Black Holes in $f(Q)$ Gravity: An RVB-Residue Approach
general relativity and quantum cosmology
This document is indexed with metadata only — full text is not available in the archive for this record.
Open the official source ↗
Record · ID 650924
Conceptio Open Knowledge Archive — every document is proof-bundled with source, license, and retrieval metadata.